Depth profile study of Pb-210 in the surface of an NaI(Tl) crystal
DC Field | Value | Language |
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dc.contributor.author | Yu, G. H. | - |
dc.contributor.author | Ha, C. | - |
dc.contributor.author | Jeon, E. J. | - |
dc.contributor.author | Kim, K. W. | - |
dc.contributor.author | Kim, N. Y. | - |
dc.contributor.author | Kim, Y. D. | - |
dc.contributor.author | Lee, H. S. | - |
dc.contributor.author | Park, H. K. | - |
dc.contributor.author | Rott, C. | - |
dc.date.accessioned | 2021-08-30T02:55:26Z | - |
dc.date.available | 2021-08-30T02:55:26Z | - |
dc.date.created | 2021-06-18 | - |
dc.date.issued | 2021-03 | - |
dc.identifier.issn | 0927-6505 | - |
dc.identifier.uri | https://scholar.korea.ac.kr/handle/2021.sw.korea/49538 | - |
dc.description.abstract | The surface Pb-210 is one of the main background sources for dark-matter-search experiments using NaI(Tl) crystals, and its spectral features associated with the beta-decay events for energies less than 60 keV depends on the depth distribution of Pb-210 in the surface of an NaI(Tl) crystal. Therefore, we must understand the profile of surface Pb-210 to precisely model the background measurement in the low-energy region for the low-background experiment using NaI(Tl) crystals. We estimate the depth profile of the surface Pb-210 contamination by modeling the measured spectrum of the alpha emission from the decay of Po-210 at the decay sequence of the surface Pb-210 contamination that is obtained using an Rn-222-contaminated crystal. In order to describe the energy spectra of the surface contamination we perform a log-likelihood fit of the measured data to a sum of Geant4 Mote Carlo simulations, weighted by an exponential curve as a function of the surface depth. The lowand high-energy events from the beta decay of surface Pb-210 are also modeled to improve the depth profile for shallow depths. We simulate the energy spectra from beta decays of Pb-210 that are exponentially distributed in the surface by following two exponential functions where the mean-depth coefficients are free parameters in the data fitting; we observed that the energy spectra are in good agreement with the measured data. (C) 2020 Elsevier B.V. All rights reserved. | - |
dc.language | English | - |
dc.language.iso | en | - |
dc.publisher | ELSEVIER | - |
dc.subject | ANOMALOUS PULSES | - |
dc.subject | DAMA/LIBRA | - |
dc.subject | MODEL | - |
dc.title | Depth profile study of Pb-210 in the surface of an NaI(Tl) crystal | - |
dc.type | Article | - |
dc.contributor.affiliatedAuthor | Park, H. K. | - |
dc.identifier.doi | 10.1016/j.astropartphys.2020.102518 | - |
dc.identifier.scopusid | 2-s2.0-85092031142 | - |
dc.identifier.wosid | 000600571200002 | - |
dc.identifier.bibliographicCitation | ASTROPARTICLE PHYSICS, v.126 | - |
dc.relation.isPartOf | ASTROPARTICLE PHYSICS | - |
dc.citation.title | ASTROPARTICLE PHYSICS | - |
dc.citation.volume | 126 | - |
dc.type.rims | ART | - |
dc.type.docType | Article | - |
dc.description.journalClass | 1 | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
dc.relation.journalResearchArea | Astronomy & Astrophysics | - |
dc.relation.journalResearchArea | Physics | - |
dc.relation.journalWebOfScienceCategory | Astronomy & Astrophysics | - |
dc.relation.journalWebOfScienceCategory | Physics, Particles & Fields | - |
dc.subject.keywordPlus | ANOMALOUS PULSES | - |
dc.subject.keywordPlus | DAMA/LIBRA | - |
dc.subject.keywordPlus | MODEL | - |
dc.subject.keywordAuthor | Surface contamination | - |
dc.subject.keywordAuthor | Depth profile | - |
dc.subject.keywordAuthor | (210) Pb | - |
dc.subject.keywordAuthor | (210) Po | - |
dc.subject.keywordAuthor | NaI(Tl) crystal | - |
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